论俯冲增生杂岩带洋板块地质构造图编图思想与方法

对地质类图件编(填)图而言,合理厘定不同级别的编(填)图单元,是保证所编(填)图件质量的关键.俯冲增生杂岩带的物质组成,主要是来自洋盆不同构造环境下洋岩石圈的构造-岩石建造,可区分出洋脊建造(蛇绿岩)、深海平原建造、洋岛(OIB)-海山建造、洋内弧建造、海沟建造、源自洋岩石圈的高压-超高压岩石建造.另外,还有混入到俯冲增生杂岩带但不源自洋岩石圈,而是源自陆岩石圈的裂离地块建造、高压-超高压岩石建造、陆缘岩浆弧建造和楔顶盆地建造等.因此,查清并厘定出不同来源的地质体建造,是开展俯冲增生杂岩带编(填)图单元划分与图件编绘的基石.本文从区分出俯冲增生杂岩带内不同来源物质建造之科学目标为出发点,将它们的编图单元划分为3级:俯冲增生杂岩带(一级单元)、岩片(二级单元)、岩块和基质(三级单元).对各级编(填)图单元类型进行了具体划分和命名,规定了其代号、用色和岩性花纹的使用要求.简述了俯冲增生杂岩带构造形变的图面表达要求,强调俯冲期和碰撞期的构造变形是俯冲增生杂岩带的两大主期变形,必须合理编(填)绘.     

西藏玛依岗日印支期增生杂岩透入性石英脉的变形期次及流体包裹体特征

造山带浅变质碎屑杂岩变质变形期次的建立有助于厘定增生杂岩的形成机制,约束洋壳俯冲带增生折返的构造过程。采用中小尺度构造解析的方法对羌塘中部玛依岗日地区的印支期增生杂岩进行剖析,发现其构造样式主要为三叠纪洋壳俯冲期E—W向单剪变形和汇聚期N—S向挤压变形的共轴叠加,并受到了新生代浅层次近南北向纵弯褶皱的轻微改造,岩石普遍发育三期构造面理,前两期伴随有浅变质作用。碎屑岩第一期剪切型流劈理S1在区域上表现为透入性的同构造压溶石英脉条带,利用流体包裹体显微测温实验,发现石英包含大量原生不混溶沸腾包裹体群,分为富CO_2三相包裹体和NaCl-H_2O气液两相包裹体,300~400℃的完全均一温度代表第一期变形的温度,非沸腾气液两相包裹体盐度-P/T等容线相图显示均值集中在0.3GPa左右,指示第一期变形的深度为~11km。增生杂岩的进变质作用不具有同一变质相系,P-T-t轨迹表现为折线式,俯冲通道浅部为中P/T变质相系,中深部为高P/T变质相系。高压变质岩折返的退变质作用具有冷却型P-T-t轨迹,晚三叠世(211~221 Ma)与浅变质杂岩发生构造拼贴,古特提斯洋同时发生关闭,羌北地块与羌南地块的短暂汇聚引起了第二期强挤压变形和同碰撞型岩浆侵入事件。     

洋板块地层学的概念、模式、组成及失序变化*

着重介绍了洋板块地层的概念、模式、组成及失序变化特征。造山带混杂岩和大陆边缘增生复合体是经历俯冲碰撞消亡后的古洋沉积记录,利用微体古生物地层学和同位素年代学方法可以重建造山带混杂岩和大陆边缘增生复合体的原始地层。洋板块地层(学)是用来描述沉淀在洋壳基底之上的沉积岩和火成岩序列的术语,其开始于洋中脊形成,终止于该洋中脊被移入到汇聚边缘增生楔。从造山带混杂岩中重建的古大洋地层的基本组成大体相似,但因大洋岩石圈的岩浆背景不同,造成不同时期和不同类型的洋板块地层组成也会有差异。在前人研究成果的基础上, 笔者通过对不同类型洋板块地层进行分类,介绍了如何从经历碰撞造山过程的增生造山带进行洋板块地层的重建。引入“洋板块地层学”概念的主要目的在于通过对因俯冲增生而消亡的具有洋壳基底的构造洋盆和边缘海盆地的地层单元进行重建,恢复已消失洋的地层组成单元,这对造山带地层解析、造山带构造古地理恢复、重大构造变革期古地理学研究和板块重建等都将起到积极的促进作用。     

黑龙江省东部跃进山增生杂岩的形成时代和构造意义

那丹哈达地体中的跃进山和饶河增生杂岩对于重建古太平洋板块的俯冲—增生过程以及揭示古太平洋和古亚洲洋之间的构造体制转换过程提供了重要地质证据。然而古太平洋板块俯冲至欧亚大陆下的起始时间以及跃进山增生杂岩相关的古洋盆属性存在较大争议。本文对跃进山增生杂岩的野外地质调查显示其具有“基质+岩块”的物质组成特征,对其中的基质变泥质粉砂岩碎屑锆石U- Pb定年结果显示其沉积时代不早于233. 1 ± 5. 1 Ma,绿片岩岩块的锆石U- Pb定年结果显示其原岩的结晶年龄为194. 7 ± 4. 8 Ma,并具有洋岛玄武岩的地球化学属性。结合前人新近发表的跃进山地区和区域上增生杂岩的岩块和基质的年代学资料,表明跃进山增生杂岩的增生时代主体为三叠纪,而最终就位时代为早侏罗世早期,它为古太平洋板块俯冲—增生的物质记录。     

On the biostratigraphy of accretionary complexes in the Far East (critical review of several papers)

Being a relatively simple geological discipline, biostratigraphy requires accuracy and sequential logic. The incorrect use of the biostratigraphic method and inaccurate interpretation of biostratigraphic data lead to a distorted understanding of regional tectonics. Frequently occurring errors are analyzed using three recently published works on biostratigraphy of accretionary complexes in the Russian Far East as an example.     

Seismic quality factors across a bottom simulating reflector in the Makran Accretionary Prism, Arabian Sea

The hydrate-bearing sediments above the bottom simulating reflector (BSR) are associated with low attenuation or high quality factor (Q), whereas underlying gas-bearing sediments exhibit high attenuation. Hence, estimation of Q can be important for qualifying whether a BSR is related to gas hydrates and free-gas. This property is also useful for identifying gas hydrates where detection of BSR is dubious. Here, we calculate the interval Q for three submarine sedimentary layers bounded by seafloor, BSR, one reflector above and another reflector below the BSR at three locations with moderate, strong and no BSR along a seismic line in the Makran accretionary prism, Arabian Sea for studying attenuation (Q⁻¹) characteristics of sediments. Interval Q for hydrate-bearing sediments (layer B) above the BSR are estimated as 191 ± 11, 223 ± 12, and 117 ± 5, whereas interval Q for the underlying gas-bearing sediments (layer C) are calculated as 112 ± 7, 107 ± 8 and 124 ± 11 at moderate, strong and no BSR locations, respectively. The large variation in Q is observed at strong BSR. Thus Q can be used for ascertaining whether the observed BSR is due to gas hydrates, and for identifying gas hydrates at places where detection of BSR is rather doubtful. Interval Q of 98 ± 4, 108 ± 5, and 102 ± 5, respectively, at moderate, strong and no BSR locations for the layer immediately beneath the seafloor (layer A) show almost uniform attenuation.     

Deformation and fluid flow during orogeny at the palaeo-Pacific active margin of Gondwana: the Early Palaeozoic Robertson Bay accretionary complex (north Victoria Land, Antarctica)

Structural investigations, integrated with X‐ray diffraction, fluid inclusion microthermometry and oxygen‐stable isotope analyses are used to reconstruct the deformation history and the palaeo‐fluid circulation during formation of the low‐grade, turbidite‐dominated Early Palaeozoic Robertson Bay accretionary complex of north Victoria Land (Antarctica). Evidence for progressive deformation is elucidated by analysing the textural fabric of chronologically distinct, thrust‐related quartz vein generations, incrementally developed during progressive shortening and thickening of the Robertson Bay accretionary complex. Our data attest that orogenic deformation was mainly controlled by dissolution–precipitation creep, modulated by stress‐ and strain‐rate‐dependent fluid pressure cycling, associated with local and regional permeability variations induced by the distribution and evolution of the fracture network during regional thrusting. Fracture‐related fluid pathways constituted efficient conduits for episodic fluid flow. The dominant migrating fluid was pre‐to‐syn‐folding and associated with the migration of warm (160–200 °C) nitrogen‐ and carbonic (CO₂ and CH₄)‐bearing fluids. Both fluid advection and diffusive mass transfer are recognized as operative mechanisms for fluid–rock interaction and vein formation during continuous shortening. In particular, fluid–rock interaction was the consequence of dissolution–precipitation creep assisted by tectonically driven cooling fluids moving through the rock section as a result of seismic pumping. The most likely source of the migrating fluids would be the frontal part of the growing accretionary complex, where fluids from the deep levels in the hinterland are driven trough channelization operated by the thrust‐related fracture (fault) systems.     

四川理塘地区花岗闪长岩特征及其增生楔弧岩浆活动

【研究目的】通过查明理塘地区拉扎嘎山花岗闪长岩的年龄、地球化学特征,探讨花岗闪长岩形成的时代、成因及构造背景,为研究甘孜—理塘洋盆俯冲增生构造演化过程提供依据。【研究方法】选取甘孜—理塘蛇绿混杂岩带俯冲增生楔内花岗闪长岩,系统开展岩相学、LA-ICP-MS锆石U-Pb年代学和岩石地球化学研究。【研究结果】花岗闪长岩含有大量的角闪石、黑云母等铁镁矿物,局部见大量的闪长质包体和围岩捕掳体。岩体形成于晚三叠世（（207.2±1.5） Ma）,岩石属I型钙碱性准铝质花岗岩类,具富集大离子亲石元素Rb、Ba、K、Th、U,亏损高场强元素Nb、Ta、P、Zr、Ti,显示轻稀土富集、重稀土亏损的右倾式配分模式,具有Eu的负异常,是典型的火山弧型花岗岩。【结论】结合区域地质资料及本文研究成果,认为四川理塘地区拉扎嘎山花岗闪长岩与甘孜—理塘洋向西俯冲致使中咱地块东缘增生楔不断扩大密切相关,是增生楔杂岩熔融成不同类型岩浆混合的产物。创新点：四川理塘地区拉扎嘎山花岗岩形成于晚三叠世,具典型的火山弧型花岗岩地球化学特征,形成于甘孜—理塘洋西向俯冲致使增生楔杂岩熔融,为甘孜—理塘洋俯冲增生构造演化提供了新的证据。     

Designating tectonostratigraphic terranes versus mapping rock units in subduction complexes: perspectives from the Franciscan Complex of California,USA

Accretionary complex histories are broadly understood. Sedimentation in seafloor and trench environments on drifting subducting plates and in associated trenches, followed by (1) deformation and metamorphism in the subduction zone and (2) subsequent uplift at the overriding plate edge, result in complicated stratigraphic and structural sequences in accretionary complexes. Recognizing, defining, and designating individual terranes in subduction complexes clarify some of these complicated relationships within the resulting continent-scale orogenic belts. Terrane designation does not substitute for detailed stratigraphic and structural mapping. Stratigraphic and structural mapping, combined with radiometric and palaeontologic dating, are necessary for delineation of coherent, broken, and dismembered formations, and various mélange units, and for clarification of the details of subduction complex architecture and history. The Franciscan Complex is a representative subduction complex that has evolved through sedimentation, faulting, folding, and low-temperature metamorphism, followed by uplift, associated deformation, and later overprinted deformation. Many belts of Franciscan rocks are offset by strike-slip faults associated with the dextral San Andreas Fault System. In the Franciscan Complex, among the terrane names applied widely, are the ‘Yolla Bolly Terrane’ and the ‘Central Terrane’. Where detailed mapping and detrital zircon ages exist, data reveal that the two names have been applied to rocks of similar general character and age. In the northeastern Diablo Range, Franciscan Complex rocks include coherent units, broken and dismembered formations, and various types of mélanges, all assigned at various times to the Yolla Bolly and other terranes. The details of stratigraphic and structural history revealed by large-scale mapping and radiometric dating prove to be more useful in clarifying the accretionary complex history than assigning a terrane name to the rocks. That history will assist in resolving terrane assignment issues and allow discrimination of subduction-associated and post-subduction events, essential for understanding the overall history of the orogen.     

OPS mélange: a new term for mélanges of convergent margins of the world

Ocean plate stratigraphy (OPS) is essential to understanding accretionary wedges and complexes along convergent plate margins. Mélanges within accretionary wedges and complexes are the products of fragmentation and mixing processes during and following OPS accretion. A new term, ‘OPS mélange’, is proposed here for mélanges composed mostly of blocks of OPS with an argillaceous matrix, and for a mixture of mélanges of multiple origins with either broken or coherent formations. An OPS mélange results from the fragmentation and disruption of OPS, without admixing of other components. Three major types of OPS mélange can be distinguished on the basis of their components: turbidite type, chert–turbidite type, and limestone–basalt type. These three types potentially form similar mélanges, but they are derived from different parts of the OPS, depending on the level of the decollement surface. The concept of ‘OPS mélange’ can be applied to most of the mélanges in accretionary prisms and complexes worldwide. In addition, this proposal recognizes a distinction between processes of fragmentation and mixing of OPS components, and mixing of ophiolite components, the latter of which results in serpentinite mélanges, not OPS mélanges. Mélanges composed of OPS sequences occur worldwide. The recognition of OPS mélanges is a key aspect of understanding tectonic processes at convergent margins, which result in mélange formation in orogenic belts globally.